One can find that the pressure (REF ) in SNM could safely pass through its empirical constraining band from analyzing the collective flow data in relativistic heavy-ion collisions [1]}, see the left panel of Fig. REF . In addition, the expression for the single-nucleon potential at the saturation density in SNM is very simple, i.e.,
\(U_0(\rho _0,\mathbf {k})=\alpha +\beta +\lambda +\phi +\mu \left\bad.\left(1+\frac{\theta |\mathbf {k}|^3}{\Lambda ^3}\right)\right..\) 
